XMM-Newton Observations of PSR B1823–13: An Asymmetric Synchrotron Nebula around a Vela-like Pulsar
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V. Kaspi | N. Schulz | B. Gaensler | Mpe | M. Pivovaroff | W. Becker | Uc Berkeley | W. B. H. CfA | V. Kaspi | B. Gaensler | Norbert S. Schulz | Mit | U. McGill
[1] V. Kaspi,et al. An X-ray Nebula Associated with the Millisecond Pulsar B1957+20 , 2003, Science.
[2] B. Stappers,et al. An Optical Bow Shock around the Nearby Millisecond Pulsar J2124–3358 , 2002, astro-ph/0210543.
[3] P. Slane,et al. Neutron Stars in Supernova Remnants , 2002 .
[4] Cambridge,et al. XMM-Newton observation of the distant (z=0.6}) galaxy cluster RX J1120.1+4318 , 2002, astro-ph/0204306.
[5] R. S. Warwick,et al. X-ray background measurements with XMM-Newton EPIC , 2002, astro-ph/0204147.
[6] N. Bucciantini. Pulsar bow-shock nebulae. II. Hydrodynamical simulation , 2002, astro-ph/0203504.
[7] G. Tóth,et al. Pulsar wind nebulae in supernova remnants Spherically symmetric hydrodynamical simulations , 2001 .
[8] V. Dwarkadas. Interaction of Supernova Remnants With the Ambient medium , 2001 .
[9] Tokyo Institute of Technology,et al. Chandra Imaging of the X-Ray Nebula Powered by Pulsar B1509–58 , 2001, astro-ph/0110454.
[10] V. Kaspi,et al. X-Ray Detection of Pulsar PSR B1757–24 and Its Nebular Tail , 2001, astro-ph/0110188.
[11] M. Colpi,et al. Re-examining the X-ray versus spin-down luminosity correlation of rotation powered pulsars , 2001, astro-ph/0109452.
[12] S. Ransom,et al. Discovery of X-Ray Pulsations from the Compact Central Source in the Supernova Remnant 3C 58 , 2001, astro-ph/0108489.
[13] G. Vasisht,et al. Chandra X-Ray Observations of G11.2–0.3: Implications for Pulsar Ages , 2001, astro-ph/0107292.
[14] J. Blondin,et al. Pulsar Wind Nebulae in Evolved Supernova Remnants , 2001, astro-ph/0107076.
[15] F. Camilo,et al. X-Ray Observations of the New Pulsar-Supernova Remnant System PSR J1119–6127 and Supernova Remnant G292.2–0.5 , 2001, astro-ph/0102084.
[16] J. Hughes,et al. RX J0852.0–4622: Another Nonthermal Shell-Type Supernova Remnant (G266.2–1.2) , 2000, astro-ph/0010510.
[17] D. Helfand,et al. Vela Pulsar and Its Synchrotron Nebula , 2000, astro-ph/0007310.
[18] D. Frail,et al. A large age for the pulsar B1757-24 from an upper limit on its proper motion , 2000, Nature.
[19] Furman,et al. Limits on radio emission from pulsar wind nebulae , 2000, astro-ph/0004273.
[20] O'Dell,et al. Discovery of Spatial and Spectral Structure in the X-Ray Emission from the Crab Nebula , 2000, The Astrophysical journal.
[21] M. Kramer,et al. IAU Colloquium 177: Pulsar Astronomy: 2000 and Beyond , 2000 .
[22] F. Pacini. Neutron Stars in Supernova Remnants , 1999, astro-ph/9911418.
[23] J. Hughes,et al. Nonthermal X-Ray Emission from the Shell-Type Supernova Remnant G347.3–0.5 , 1999 .
[24] S. Reynolds,et al. Maximum Energies of Shock-accelerated Electrons in Young Shell Supernova Remnants , 1999 .
[25] Ulrich G. Briel,et al. Time resolution capability of the XMM EPIC pn-CCD in different readout modes , 1999, Optics & Photonics.
[26] A. Harding,et al. A Rossi X-Ray Timing Explorer Observation of the Vela Pulsar: Filling in the X-Ray Gap , 1999, astro-ph/9904357.
[27] D. Helfand,et al. ASCA Observations of the Composite Supernova Remnant G29.7-0.3 , 1996 .
[28] J. Finley,et al. The morphology of young neutron stars: PSR B1823-13, its compact nebula, and its interstellar neighborhood , 1996 .
[29] R. Petre,et al. Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006 , 1995, Nature.
[30] D. Frail,et al. Does the Crab Have a Shell? , 1995, astro-ph/9509135.
[31] Zhi-Yun Li,et al. The X-ray-emitting trail of the nearby pulsar PSR1929 + 10 , 1993, Nature.
[32] P. Bodenheimer,et al. On the evolution of supernova remnants. III. Off-centred supernova explosions in pre-existing wind-driven bubbles. , 1993 .
[33] D. McCammon,et al. Photoelectric absorption cross sections with variable abundances , 1992 .
[34] A. Lyne,et al. A high-frequency survey of the galactic plane for young and distant pulsars. , 1992 .
[35] P. Bodenheimer,et al. On the evolution of supernova remnants. I. Explosions inside pre-existing wind-driven bubbles. , 1990 .
[36] W. Goss,et al. Three Fields Containing Young Pulsars: The Observable Lifetime of Supernova Remnants , 1989 .
[37] S. Reynolds,et al. No shell around 3C 58 , 1985 .
[38] C. Kennel,et al. Confinement of the Crab pulsar's wind by its supernova remnant , 1984 .
[39] D. Leahy,et al. On searches for periodic pulsed emission - The Rayleigh test compared to epoch folding , 1983 .
[40] S. Reynolds,et al. Evolution of pulsar-driven supernova remnants , 1981 .
[41] Barham W. Smith,et al. Soft X-ray spectrum of a hot plasma. , 1977 .
[42] M. Kramer,et al. Pulsar Astronomy - 2000 and Beyond , 2000 .